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In FLWR metric or in Minkowski metric or in any general metric can we say that ##ds^2=0## cause speed of light should be constant to all observers ?
Or there's another reason ?
Or there's another reason ?
Arman777 said:In FLRW metric when we measure the redshift we assume ##ds^2=0##.
Like also in minkowski metric ##ds^2=0## cause only in that case we can get c=dx/dt.
Probably I should add to the question why for a light ##ds^2=0##...
Orodruin said:This is not a measurement of redshift. It is a computation of the redshift based on the FLRW universe. Studying light, it is quite clear that we must use a light-like geodesics.
The redshift you are talking about is for light. Light travels on null geodesics. Therefore ##ds^2=0##. It is not a general statement about the metric, it is a specific statement about light.Arman777 said:In FLRW metric when we measure the redshift we assume ds2=0ds2=0ds^2=0.
Same thing here. For light ##ds^2=0## for the reason you gave. But for massive objects ##ds^2<0## and for hypothetical tachyons ##ds^2>0##.Arman777 said:Like also in minkowski metric ds2=0ds2=0ds^2=0 cause only in that case we can get c=dx/dt.
If you write down the metric, set ##ds^2=0##, then what are you left with? The equation of a sphere of radius ##ct##. This is something traveling at c in all directions, which is the second postulate. Therefore, ##ds^2=0## for light is the mathematical statement of the second postulate.Arman777 said:Probably I should add to the question why for a light ds2=0ds2=0ds^2=0...
I think it should be qualified that whether ##ds^2 > 0## or ##ds^2 < 0## for time-like world lines depends on the sign convention for the metric. Mathematicians and GR people generally prefer ##ds^2 < 0## while particle physicists prefer ##ds^2 > 0##. Always check which convention is being used in the particular text. Of course, this does not affect ##ds^2 = 0## for null world lines.Dale said:Same thing here. For light ##ds^2=0## for the reason you gave. But for massive objects ##ds^2<0## and for hypothetical tachyons ##ds^2>0##.
Yes, good point. My preferred convention is to write ##ds^2## when I am using the (-+++) convention and to write ##d\tau^2## when I am using the (+---) conventionOrodruin said:I think it should be qualified that whether ds2>0ds2>0ds^2 > 0 or ds2<0ds2<0ds^2 < 0 for time-like world lines depends on the sign convention for the metric.
Yes I tried to mean that, as I understood from your post for light ##ds^2=0##. But Is this true for all of the metrics ?Dale said:It is not a general statement about the metric, it is a specific statement about light.
I see, thanksDale said:If you write down the metric, set ds2=0ds2=0ds^2=0, then what are you left with? The equation of a sphere of radius ctctct. This is something traveling at c in all directions, which is the second postulate. Therefore, ds2=0ds2=0ds^2=0 for light is the mathematical statement of the second postulate.
I understand it nowOrodruin said:Light is massless and moves along null geodesics.
Yes, it is true for all metrics and all spacetimesArman777 said:But Is this true for all of the metrics ?
Thanks a lotDale said:Yes, it is true for all metrics and all spacetimes
The value of ds^2 being equal to 0 in metrics is a result of the metric tensor, which measures the distance between two points in a given space. In certain cases, such as in a flat or empty space, the metric tensor is defined as ds^2 = dx^2 + dy^2 + dz^2, leading to a value of 0.
In metrics, ds^2 represents the squared distance between two points in a given space. This is calculated using the metric tensor, which is a mathematical tool used to measure distances and angles in a particular space.
In the theory of relativity, ds^2 is used to calculate spacetime intervals, which represent the distance between two events in spacetime. This is done by taking the square root of the difference between the squared space interval (dx^2 + dy^2 + dz^2) and the squared time interval (c^2dt^2).
Yes, in certain cases, ds^2 can be negative in metrics. This occurs in spaces with a negative curvature, such as in the theory of general relativity, where the metric tensor is defined as ds^2 = -dt^2 + dx^2 + dy^2 + dz^2.
The value of ds^2 has a direct impact on the geometry of a space. In spaces with a positive value of ds^2, known as Euclidean spaces, the geometry is flat and follows the rules of Euclidean geometry. In spaces with a negative value of ds^2, known as non-Euclidean spaces, the geometry is curved and follows the rules of non-Euclidean geometry.